Long gamma-ray burst rate at very high redshift

Abstract

Future missions for long gammma-ray burst (GRB) observations at high redshift such as HiZ-GUNDAM and THESEUS will provide clue to the star formation history in our universe. In this paper focusing on high redshift (z>8) GRBs, we calculate the detection rate of long GRBs by future observations, considering both Population (Pop) I&II stars and Pop III stars as GRB progenitors. For the Pop I&II star formation rate (SFR), we adopt an up-to-date model of high-redshift SFR based on the halo mass function and dark matter accretion rate obtained from cosmological simulations. We show that the Pop I&II GRB rate steeply decreases with redshift. This would rather enable us to detect the different type of GRBs, Pop III GRBs, at very high redshift. If 10% or more Pop III stars die as an ultra-long GRB, the future missions would detect such GRBs in one year in spite of their low fluence. More luminous GRBs are expected from massive compact Pop III stars produced via the binary merger. In our conventional case, the detection rate of such luminous GRBs is 3-20 /yr (z>8). Those future observations contribute to revealing of the Pop III star formation history.

arXiv commentcomments welcome. Accepted to ApJ

References in corpus (81)

• Planck 2015 results. XIII. Cosmological parameters
• Planck 2013 results. XVI. Cosmological parameters
• Cosmic Star Formation History
• Large scale bias and the peak background split
• The Average Star Formation Histories of Galaxies in Dark Matter Halos from z=0-8
• Binary interaction dominates the evolution of massive stars
• Discovery of the peculiar supernova 1998bw in the error box of GRB980425
• Comprehensive analytic formulae for stellar evolution as a function of mass and metallicity
• Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Likelihoods and Parameters from the WMAP data
• A very energetic supernova associated with the gamma-ray burst of 29 March 2003
• The Formation of the First Star in the Universe
• UV Luminosity Functions at redshifts z~4 to z~10: 10000 Galaxies from HST Legacy Fields
• Binary Black Hole Mergers in the first Advanced LIGO Observing Run
• The Formation of the First Stars. I. The Primordial Star Forming Cloud
• Common Envelope Evolution: Where we stand and how we can move forward
• Halos and galaxies in the standard cosmological model: results from the Bolshoi simulation
• The Progenitor Stars of Gamma-Ray Bursts
• How small were the first cosmological objects?
• Astrophysical Implications of the Binary Black-Hole Merger GW150914
• Pulsational pair instability as an explanation for the most luminous supernovae
• Evolution of rapidly rotating metal-poor massive stars towards gamma-ray bursts
• One Hundred First Stars : Protostellar Evolution and the Final Masses
• The VLT-FLAMES Tarantula Survey VIII. Multiplicity properties of the O-type star population
• Single star progenitors of long gamma-ray bursts I: Model grids and redshift dependent GRB rate
• Thermal and Fragmentation Properties of Star-forming Clouds in Low-metallicity Environments
• Formation of Primordial Stars in a LCDM Universe
• A Photometric Redshift of z ~ 9.4 for GRB 090429B
• Protostellar Feedback Halts the Growth of the First Stars in the Universe
• The Dearth of z~10 Galaxies in all HST Legacy Fields -- The Rapid Evolution of the Galaxy Population in the First 500 Myr
• The Effect of Pair-Instability Mass Loss on Black Hole Mergers
• The luminosity function and the rate of Swift's Gamma Ray Bursts
• The Mass Spectrum of the First Stars
• Possible Indirect Confirmation of the Existence of Pop III Massive Stars by Gravitational Wave
• A new population of ultra-long duration gamma-ray bursts
• Post-common-envelope binaries from SDSS. IX: Constraining the common-envelope efficiency
• The Star Formation Rate in the Reionization Era as Indicated by Gamma-ray Bursts
• The Formation of the First Stars II. Radiative Feedback Processes and Implications for the Initial Mass Function
• High-Redshift Gamma-Ray Bursts from Population III Progenitors
• Evolution of massive population III stars with rotation and magnetic fields
• A Comprehensive Analysis of Swift/XRT Data: III. Jet Break Candidates in X-ray and Optical Afterglow Lightcurves
• The THESEUS space mission concept: science case, design and expected performances
• The ultra-long Gamma-Ray Burst 111209A: the collapse of a blue supergiant?
• The First Billion Years project - III: The impact of stellar radiation on the coevolution of Populations II and III
• Predictions for mass-loss rates and terminal wind velocities of massive O-type stars
• The cooling of shock-compressed primordial gas
• Constraining the Statistics of Population III Binaries
• Stellar evolution with rotation XIII: Predicted GRB rates at various Z
• A Simple Technique for Predicting High-Redshift Galaxy Evolution
• Cosmological Aspects of Gamma-Ray Bursts: Luminosity Evolution and an Estimate of the Star Formation Rate at High Redshifts
• Gravitational Waves from the Remnants of the First Stars
• Binary Merger Progenitors for Gamma-Ray Bursts and Hypernovae
• An Unexpectedly Swift Rise in the Gamma-ray Burst Rate
• GOLDRUSH. II. Clustering of Galaxies at $z\sim 4-6$ Revealed with the Half-Million Dropouts Over the 100 deg${}^2$ Area Corresponding to 1 Gpc${}^3$
• Evolution of Stellar-to-Halo Mass Ratio at z=0-7 Identified by Clustering Analysis with the Hubble Legacy Imaging and Early Subaru/Hyper Suprime-Cam Survey Data
• Population III.1 and III.2 gamma-Ray Bursts: Constraints on the event rate for future radio and X-ray surveys
• The detection rate of Inspiral and Quasi-normal modes of Pop III binary black holes which can confirm or refute the General Relativity in the strong gravity region
• Can Gamma-Ray Burst Jets Break Out the First Stars?
• Probing the Cosmic Gamma-Ray Burst Rate with Trigger Simulations of the Swift Burst Alert Telescope
• Blue Supergiant Model for Ultra-Long Gamma-Ray Burst with Superluminous-Supernova-Like Bump
• Population III GRB Afterglows: Constraints on Stellar Masses and External Medium Densities
• Double-core evolution and the formation of neutron-star binaries with compact companions
• Gravitational wave background from Population III binary black holes consistent with cosmic reionization
• Population III stars and the Long Gamma Ray Burst rate
• Conditions for the Formation of First-Star Binaries
• Diversity of GRB energetics vs. SN homogeneity: supernova 2013cq associated with the gamma-ray burst 130427A
• The ${\nu }^2$GC Simulations : Quantifying the Dark Side of the Universe in the Planck Cosmology
• Limits on Population III star formation in minihaloes implied by Planck
• Protostellar Feedback and Final Mass of the Second-Generation Primordial Stars
• The winds of the hot massive first stars
• Discovery of Radio Afterglow from the Most Distant Cosmic Explosion
• Accessing the population of high redshift Gamma Ray Bursts
• Long Duration X-Ray Flash and X-Ray Rich Gamma Ray Burst from Low Mass Population III Star
• The Formation of Population III Binaries
• The Lack of Gamma-Ray Bursts from Population III Binaries
• Perspectives on Gamma-Ray Burst Physics and Cosmology with Next Generation Facilities
• CNO driven winds of hot first stars
• Gamma-ray bursts and Population III stars
• Gamma-ray bursts from massive Population III stars: clues from the radio band
• The possible existence of Pop III NS-BH binary and its detectability
• Long gamma ray burst rate in the binary merger progenitor model
• Development of wide-field low-energy X-ray imaging detectors for HiZ-GUNDAM

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• On the Cosmological Evolution of Long Gamma-ray Burst Properties
• Probing the initial mass function of the first stars with transients
• High Redshift Long Gamma-Ray Bursts Hubble Diagram as a Test of Basic Cosmological Relations
• The 21-cm forest as a simultaneous probe of dark matter and cosmic heating history
• Gamma-Ray Bursts with Extended Emission: Classifications, Energy Correlations and Radiation Properties
• The most massive Population III stars
• Ultra-Long Gamma-Ray Bursts detection with SVOM/ECLAIRs
• The Consequences of Gamma-ray Burst Jet Opening Angle Evolution on the Inferred Star Formation Rate
• Fires in the deep: The luminosity distribution of early-time gamma-ray-burst afterglows in light of the Gamow Explorer sensitivity requirements
• A Global Semi-Analytic Model of the First Stars and Galaxies Including Dark Matter Halo Merger Histories
• Large-scale asymmetry between clockwise and counterclockwise galaxies revisited
• GRBs luminosity function synthesized from \textit{Swift/BAT}, \textit{Fermi/GBM} and \textit{Konus-Wind} data
• Black Hole - Neutron Star and Binary Neutron Star Mergers from Population III and II stars
• Analytical modeling of the one-dimensional power spectrum of 21-cm forest based on a halo model method
• From Dark Matter Minihalos to Large-Scale Radiative Feedback: A Self-Consistent 3D Simulation of the First Stars and Galaxies using Neural Networks